Please use this identifier to cite or link to this item: http://hdl.handle.net/2440/127618
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dc.contributor.authorDavis, D.en
dc.contributor.authorTroiano, M.en
dc.contributor.authorChinnici, A.en
dc.contributor.authorSaw, W.en
dc.contributor.authorLau, T.en
dc.contributor.authorSolimene, R.en
dc.contributor.authorSalatino, P.en
dc.contributor.authorNathan, G.en
dc.date.issued2019en
dc.identifier.citationSolar Energy, 2019; 190:126-138en
dc.identifier.issn0038-092Xen
dc.identifier.urihttp://hdl.handle.net/2440/127618-
dc.description.abstractWe present the first experimental assessment of the influence of receiver tilt angle on the particle residence time distribution (RTD) of a two-phase solar particle receiver. The tracer pulse response method is used to measure the particle RTD within a laboratory-scale vortex-based solar particle receiver, with the particle phase itself used as the tracer. The experimental parameters of particle size, transporting gas inlet velocity and a range of receiver tilt angles – spanning 180° from vertically upward to downward facing – were systematically varied to determine the influence of key controlling parameters on the particle RTD within the receiver. It was found that the Stokes number of the two-phase flow evaluated at the receiver outlet, Sk(out), has a controlling influence on the residence time and that the influence of the receiver tilt angle is significant for large particles (Sk(out) > 10) but weak for small particles (Sk(out) ~ 1). This implies that it is preferable to operate tower-mounted systems (i.e. with downward facing receiver tilt angles) with Sk(out) ~ 1. Furthermore, a preliminary scale-up assessment suggests that the influence of tilt angle on the residence time of particles 200 µm and smaller will be insignificant for a nominal 50 MW-scale receiver, which will provide flexibility in the design of industrial-scale devices. Finally, the residence time behaviour for the range of tilt angles assessed can be well described by an analytical compartment model consisting of a small plug flow reactor, followed by two continuously-stirred tank reactors in parallel with a second plug flow reactor.en
dc.description.statementofresponsibilityDominic Davis, Maurizio Troiano, Alfonso Chinnici, Woei L. Saw, Timothy Lau, Roberto Solimene, Piero Salatino, Graham J. Nathanen
dc.language.isoenen
dc.publisherElsevieren
dc.rights© 2019 International Solar Energy Society. Published by Elsevier Ltd. All rights reserved.en
dc.subjectSolar particle receiver; vortex flow; residence time; RTD; tilt angle; CSTen
dc.titleParticle residence time distributions in a vortex-based solar particle receiver-reactor: the influence of receiver tilt angleen
dc.typeJournal articleen
dc.identifier.rmid0030132748en
dc.identifier.doi10.1016/j.solener.2019.07.078en
dc.identifier.pubid491731-
pubs.library.collectionMechanical Engineering publicationsen
pubs.library.teamDS14en
pubs.verification-statusVerifieden
pubs.publication-statusPublisheden
dc.identifier.orcidDavis, D. [0000-0001-7037-5447]en
dc.identifier.orcidChinnici, A. [0000-0002-0743-3904]en
dc.identifier.orcidSaw, W. [0000-0002-2538-5811]en
dc.identifier.orcidLau, T. [0000-0003-1851-706X]en
dc.identifier.orcidNathan, G. [0000-0002-6922-848X]en
Appears in Collections:Mechanical Engineering publications

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